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VG1 SAT LECP CALIBRATED RESAMPLED SECTORED 15MIN V1.0

This data set consists of resampled data from the Low Energy Charged Particle (LECP) experiment on Voyager 1 while the spacecraft was in the vicinity of Saturn. This instrument measures the intensities of in-situ charged particles (>26 keV electrons and >30 keV ions) with various levels of discrimination based on energy, mass species, and angular arrival direction. A subset of almost 100 LECP channels are included with this data set. The LECP data are globally calibrated to the extent possible (see below) and they are time averaged to about 15 minute time intervals with the exact beginning and ending times for those intervals matching the LECP instrumental cycle periods (the angular scanning periods).

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MAVEN SWIA Calibrated Coarse Survey 3D Data Collection

SWIA coarse survey 3d files with time-ordered fully calibrated ion distributions in units of differential energy flux derived from the SWIA Coarse distribution Survey telemetry, as well as a header of ancillary information needed to interpret the data. Description of the SWIA instrument can be found on the SWIA home page https://lasp.colorado.edu/maven/science/instrument-package/swia/ and in the SWIA instrument publication https://doi.org/10.1007/s11214-013-0029-z.

NEW HORIZONS SWAP PLUTO CRUISE CALIBRATED V3.0

This data set contains Calibrated data taken by the New Horizons Solar Wind Around Pluto instrument during the pluto cruise mission phase. This is VERSION 3.0 of this data set. Per the original mission plan for cruise operations, the SWAP instrument was off for the first 460+ days of Pluto Cruise. After that the operations were sporadic (just a few days in 2009) and mostly Science, alternating with Channel Electron Multiplier gain tests during Annual CheckOuts. After extensive testing in early 2012, in July of that year the project approved daily science operations for the SWAP and PEPSSI instruments throughout the rest of the cruise to Pluto. The changes in Version 3.0 were re-running of the ancillary data in the data product, updated geometry from newer SPICE kernels, minor editing of the documentation, catalogs, etc., and resolution of liens from the December, 2014 review, plus those from the May, 2016 review of the Pluto Encounter data sets. New observations added with this version (V3.0) include ongoing cruise observations from August, 2014 through January, 2015.

EPOXI EARTH OBS - HRIV CALIBRATED IMAGES V2.0

This data set contains calibrated, narrow band filter images (350-950 nm) of Earth acquired by the Deep Impact High Resolution Visible CCD (HRIV) during the EPOCh and Cruise 2 phases of the EPOXI mission. Five sets of observations were acquired on 18-19 March, 28-29 May and 04-05 June 2008 and on 27-28 March and 04-05 October 2009 to characterize Earth as an analog for extrasolar planets. Each observing period lasted approximately 24 hours. HRIV images were acquired once per hour with the filters centered on 350, 750 and 950 nm, whereas the 450-, 550-, 650-, and 850-nm data were taken every 15 minutes. During the observing period in May 2008, the Moon transited across Earth as seen from the spacecraft. On 27 September 2009 during the first attempt of an Earth south polar observation, only seven HRIV frames were acquired before fault protection turned that instrument off; the full sequence was successfully rerun on 04-05 October 2009. Version 2.0 includes the application of a horizontal destriping process and revised electronic crosstalk calibration files.

IHW COMET IRIMAG CALIBRATED EXPERIMENT DATA RECORD GZ V1.0

In preparation for the concerted international study of Comet Halley, the IHW conducted a trial run with observations of Comet Crommelin, largely during February and March of 1984.

NEW HORIZONS LEISA KEM1 CALIBRATED V2.0

This data set contains Calibrated data taken by the New Horizons Linear Etalon Imaging Spectral Array instrument during the KEM1 ENCOUNTER mission phase. This is VERSION 2.0 of this data set. This data set contains LEISA observations taken for functional testing, and MU69 [ASTEROID 486958 (2014 MU69)] Encounter operations, including a test of a slow scan rate. Many LEISA Composition and System Scans along with some LEISA Scans as a LORRI Rider. This data set contains data acquired by the spacecraft between 08/14/2018 and 01/31/2019. It only includes data downlinked before 02/01/2019. Future datasets may include more data acquired by the spacecraft after 08/13/2018 but downlinked after 01/31/2019.

VENUS CLIMATE ORBITER IR2 CALIBRATED DATA V1.0

The VCO IR2 CDR data set contains products acquired by the IR2 instrument onboard the Venus Climate Orbiter (VCO, also known as PLANET-C and AKATSUKI) spacecraft. The data files are provided in FITS format with an HDU as IMAGE extension, and it also contains metadata to the header of the HDU.

NEW HORIZONS MVIC KEM1 CALIBRATED V2.0

This data set contains Calibrated data taken by the New Horizons Multispectral Visible Imaging Camera instrument during the KEM1 ENCOUNTER mission phase. This is VERSION 2.0 of this data set. This data set contains data acquired by the spacecraft between 08/14/2018 and 01/31/2019. It only includes data downlinked before 02/01/2019. Future datasets may include more data acquired by the spacecraft after 08/13/2018 but downlinked after 01/31/2019. The data includes functional tests and images during the approach and departure of MU69,

ODYSSEY MARS MARIE CALIBRATED DATA V1.0

The MARIE (Martian Radiation Environment Experiment) aboard the 2001 Mars Odyssey spacecraft, was launched on April 7, 2001 and arrived at Mars on October 24, 2001. Data were collected intermittently during the cruise phase, starting in late April and ending in late July. A problem with MARIE's onboard computer occurred in early August and the instrument was turned off until early March 2002, after Odyssey's mapping orbit had been established. Data have been collected from that time to the present without major interruption. Routine minor interruptions of up to 36 hours have occurred during the orbital phase, in which the instrument's data is erased from the local storage (after having been downloaded). MARIE is oriented to point in the direction opposite Odyssey's velocity vector. Space radiation is for most part isotropic, so the orientation of Odyssey is usually not critical and references to external coordinate systems are not a part of the data returned by MARIE. There is one exception to the statement that space radiation is isotropic. During the early stages of solar particle events, there can be directionality in the particle flux.

IRTF S NSFCAM RAW AND CALIBRATED RING PLANE CROSSING V1.0

This dataset contains IRTF images of the Saturn system obtained with the NSFCam in early August 1995. The observations were made four days prior to the ring plane crossing when the sun and Earth were on opposite sides of the ring plane. The observations include sequences of rapid exposures of several satellite mutual events and spectroscopic data of the main rings and the E and G rings.

C130 EARTH ASAS CALIBRATED REDUCED DATA RECORD IMAGE V1.0

Most of the ASAS data acquired for GRSFE were taken during flights over Lunar Lake, Nevada, at a nominal altitude of 5000 m above ground level. Flights over Lunar Lake were repeated to acquire data for a range of solar zenith angles and to obtain data for several view azimuth angles (i.e., for several flight headings relative to the solar principal plane). On most flights, the sensor field of view was initially pointed forward 45 degrees as the aircraft approached the site. The sensor then imaged the site through a sequence of seven fore-to-aft view directions ranging from 45 degrees forward to 45 degrees aft in 15 degree increments as the aircraft flew over the site. The primary target of interest was the Lunar Lake playa, but the digital images also include data for the lava flow and cobble areas within and around the playa. Data were acquired in a similar manner on one flight over the Ubehebe Crater. One flight over Lunar Lake was also flown approximately along the solar principal plane with the ASAS view zenith angle fixed at the solar zenith angle. The purpose of this flight was to observe the opposition effect.

CASSINI ORBITER SATURN UVIS CALIBRATION DATA 1.1

Observations of solar or stellar targets for the purpose of calibrating detector wavelength scale, photometric sensitivity and flat fields.

EPOXI 103P/HARTLEY2 ENCOUNTER - HRII CALIBRATED SPECTRA V3.0

This dataset contains calibrated, 1.05- to 4.8-micron spectral images of comet 103/P Hartley 2 acquired by the High Resolution Infrared Spectrometer (HRII) from 01 October through 26 November 2010 during the Hartley 2 encounter phase of the EPOXI mission. Version 3.0 includes the application of scaled master dark subtraction for DOY 307 and in scene dark subtraction for DOY 311-313, as well as the use of an average per scan optical bench temperature in the pipeline processing. Version 3 also includes the calibration enhancements implemented in Version 2 of this dataset: a new per-pixel linearity correction treatment and its propagation through the calibration steps (i.e., bad-pixel maps, flat-field file update, revised spectral calibration curve), new mode-dependent master darks, an optimized scaling factor for the master dark, and a refinement in the absolute spectral calibration curve.

MMT OBSERVATORY 6.5M CLIO CALIBRATED OBSERVATIONS OF LCROSS

This archive contains calibrated observations of the 2009-10-09 impact of the LCROSS spacecraft on the moon by the CLIO instrument on the MMT Observatory 6.5m telescope. The archive consists of calibrated FITS images of the event. This is one of several data sets of Earth-based observations of the impact.

ROSETTA-ORBITER 67P RPCMAG 3 ESC4 CALIBRATED V9.0

This dataset contains CALIBRATED (CODMAC LEVEL 3) DATA of the COMET ESCORT 4 Phase from October 21, 2015 until January 12, 2016 of the ROSETTA orbiter magnetometer RPCMAG. Observations are done in the vicinity of comet 67P/CHURYUMOV-GERASIMENKO 1 (1969 R1). The current version of the dataset is V9.0. The difference to the datasets of earlier versions is mainly a significantly improved sensor temperature model, more detailed documentation about magnetic disturbance sources, more data handling information for the user and also an improved quality flagging system.

NEW HORIZONS SDC KEMCRUISE1 CALIBRATED V2.0

This data set contains Calibrated data taken by the New Horizons Student Dust Counter instrument during the CRUISE TO FIRST KBO ENCOUNTER mission phase. This is VERSION 2.0 of this data set. This data set contains data acquired by the spacecraft between 10/17/2016 and 08/13/2018. This is the complete dataset.

MER2 Pancam Science Calibrated Data Bundle

This bundle contains calibrated data from the Panoramic Cameras (Pancam) on Mars Exploration Rover 2 (Spirit). These data were produced by the science team.

EPOXI INFLIGHT CALIBRATIONS - HRIV RAW IMAGES V1.0

This data set contains raw calibration images acquired by the Deep Impact Medium Resolution Visible CCD from 04 October 2007 through 17 December 2008 for the EPOXI mission.

IHW COMET RSOC CALIBRATED EXPERIMENT DATA RECORD GZ V1.0

In preparation for the concerted international study of Comet Halley, the IHW conducted a trial run with observations of Comet Crommelin, largely during February and March of 1984.

CASSINI ORBITER SATURN UVIS CALIBRATION DATA V1.4

Observations of solar or stellar targets for the purpose of calibrating detector wavelength scale, photometric sensitivity and flat fields.